Kepler-275 is 6,635 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 6,165 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-275 b goes round its star every 10.3 days, 9 times as often as Mercury goes round the Sun.
| Surface temperature | 6,165 K |
| Mass | 1.189 solar masses |
| Radius | 1.383 solar radii |
| Luminosity | 2.814 times the Sun |
| Apparent magnitude | 15.289 |
| Age | about 3.39 billion years |
| Distance from the Sun | 6634.8 light-years (2034.2 parsecs) |
| Position (J2000) | RA 292.4797°, Dec 38.5149° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-275 b | 10.3 days | 0.0980 AU | 2.34 R⊕ | 6.08 M⊕ estimated | Transit, 2014 |
| Kepler-275 c | 16.1 days | 0.132 AU | 3.38 R⊕ | 11.4 M⊕ estimated | Transit, 2014 |
| Kepler-275 d | 35.7 days | 0.224 AU | 3.33 R⊕ | 11.1 M⊕ estimated | Transit, 2014 |
Values are the NASA Exoplanet Archive’s composite parameters. A radius marked estimated comes from a mass–radius relation; a mass marked minimum is M sin i. Planet sizes and colours in the 3D view are renderings: none of these worlds has been photographed as more than a point of light.
For a star of 6,165 K, 2.8 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.56 to 2.72 AU. None of its known planets orbits inside it. The zone says how much starlight arrives, not whether a planet has water or air. The edges follow Kopparapu et al. (2014), as the 3D view draws them.
The light you see left 6,635 years ago, around 4600 BC.